Paramonova, Olga P.Mishenina, Tamara V.Chepizhko, Oleksandr O.Парамонова, Ольга ПетрівнаМішеніна, Тамара ВасилівнаЧепіжко, Олександр Олександрович2014-03-282014-03-282013Odessa Astronomical Publicationshttps://dspace.onu.edu.ua/handle/123456789/4779The sulfur abundance was determined by the synthetic spectrum method in the stars with metallicity close to that of the Sun. The comparison with the results of other authors, as well as the nucleosynthesis computations were made.enstars: abundancestars: late-typeArticle